Azimuthally averaged surface brightness brightness profiles of the ε Eri dust disk (case “A”) at three Spitzer/MIPS wavelengths: 24 μm (top), 70 μm (middle), and 160 μm (bottom). Points with error bars: star-subtracted MIPS data (Fig. 6 of Backman et al. 2009). Solid lines: modeled profiles after convolution with the PSFs. Thin solid lines: the instrumental PSF.
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